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The Gaia-ESO Survey was designed to target all major Galactic components (i.e. bulge, thin and thick discs, halo and clusters), with the goal of constraining the chemical and dynamical evolution of the Milky Way. This paper presents the methodology and considerations that drive the selection of t...


Stonkutė, E.Koposov, S. E.Howes, L. M.Feltzing, S.Worley, C. C.Gilmore, G.Ruchti, G. R.Kordopatis, G.Randich, S.Zwitter, T.Bensby, T.Bragaglia, A.Smiljanic, R.Costado, M. T.Tautvaišienė, G.Casey, A. R.Korn, A. J.Lanzafame, A. C.Pancino, E.Franciosini, E.Hourihane, A.Jofré, P.Lardo, C.Lewis, J.Magrini, L.Monaco, L.Morbidelli, L.Sacco, G. G.Sbordone, L.[The Gaia-ESO Survey: the selection function of the Milky Way field stars]The Gaia-ESO Survey: the selection function of the Milky Way field stars

Aims. We present observations from the Gaia-ESO Survey in the lines of Hα, [N II], [S II], and He I of nebular emission in the central part of the Carina nebula. Methods. We investigate the properties of the two already known kinematic components (approaching and receding), which account for the ...


Damiani, F.Bonito, R.Magrini, L.Prisinzano, L.Mapelli, M.Micela, G.Kalari, V.Maíz Apellániz, J.Gilmore, G.Randich, S.Alfaro, E.Flaccomio, E.Koposov, S.Klutsch, A.Lanzafame, A. C.Pancino, E.Sacco, G. G.Bayo, A.Carraro, G.Casey, A. R.Costado, M. T.Franciosini, E.Hourihane, A.Lardo, C.Lewis, J.Monaco, L.Morbidelli, L.Worley, C.Zaggia, S.Zwitter, T.Dorda, R.[Gaia-ESO Survey: Gas dynamics in the Carina nebula through optical emission lines]Gaia-ESO Survey: Gas dynamics in the Carina nebula through optical emission lines

We analyze the kinematics of similar to 2000 giant stars in the direction of the Galactic bulge, extracted from the Gaia-ESO survey in the region -10 degrees less than or similar to l less than or similar to 10 degrees and -11 degrees less than or similar to b less than or similar to -3 degrees. ...


Williams, Angus A.Evans, N. W.Molloy, MatthewKordopatis, GeorgesSmith, M. C.Shen, J.Gilmore, G.Randich, S.Bensby, T.Francois, P.Koposov, S.E.Recio-Blanco, A.Bayo, A.Carraro, G.Casey, A.Costado, T.Franciosini, E.Hourihane, A.de Laverny, P.Lewis, J.Lind, K.Magrini, L.Monaco, L.Morbidelli, L.Sacco, G. GWorley, C.Zaggia, S.Mikolaitis, Š.[THE GAIA-ESO SURVEY: METAL-RICH BANANAS IN THE BULGE]THE GAIA-ESO SURVEY: METAL-RICH BANANAS IN THE BULGE

Smiljanic, R.Franciosini, E.Randich, S.Magrini, L.Bragaglia, A.Pasquini, L.Vallenari, A.Tautvaišienė, G.Biazzo, K.Frasca, A.Donati, P.Delgado Mena, E.Casey, A. R.Geisler, D.Villanova, S.Tang, B.Sousa, S. G.Gilmore, G.Bensby, T.François, P.Koposov, S. E.Lanzafame, A. C.Pancino, E.Recio-Blanco, A.Costado, M. T.Hourihane, A.Lardo, C.de Laverny, P.Lewis, J.Monaco, L.Morbidelli, L.Sacco, G. G.Worley, C. C.Zaggia, S.Martell, S.[The Gaia-ESO Survey: Inhibited extra mixing in two giants of the open cluster Trumpler 20?]The Gaia-ESO Survey: Inhibited extra mixing in two giants of the open cluster Trumpler 20?

We present the abundance analysis for a sample of 18 red giant branch stars in the metal-poor globular cluster NGC 4147 based on medium- and high-resolution spectra. This is the first extensive spectroscopic study of this cluster. We derive abundances of C, N, O, Na, Mg, Al, Si, Ca, Ti, Cr, Fe, N...


Villanova, S.Monaco, L.Moni Bidin, C.Assmann, P.[A spectroscopic study of the globular Cluster NGC 4147]A spectroscopic study of the globular Cluster NGC 4147

Rojas-Arriagada, A.Recio-Blanco, A.de Laverny, P.Schultheis, M.Guiglion, G.Mikolaitis, Š.Kordopatis, G.Hill, V.Gilmore, G.Randich, S.Alfaro, E. J.Bensby, T.Koposov, S. E.Costado, M. T.Franciosini, E.Hourihane, A.Jofré, P.Lardo, C.Lewis, J.Lind, K.Magrini, L.Monaco, L.Morbidelli, L.Sacco, G. G.Worley, C. C.Zaggia, S.Chiappini, C.[The Gaia-ESO Survey: Separating disk chemical substructures with cluster models⋆ Evidence of a separate evolution in the metal-poor thin disk]The Gaia-ESO Survey: Separating disk chemical substructures with cluster models⋆ Evidence of a separate evolution in the metal-poor thin disk

Context. Rapidly rotating, low-mass members of eclipsing binary systems have measured radii that are significantly larger than predicted by standard evolutionary models. It has been proposed that magnetic activity is responsible for this radius inflation. Aims. By estimating the radii of low-ma...


Jackson, R. J.Jeffries, R. D.Randich, S.Bragaglia, A.Carraro, G.Costado, M. T.Flaccomio, E.Lanzafame, A. C.Lardo, C.Monaco, L.Morbidelli, L.Smiljanic, R.Zaggia, S.[The Gaia-ESO Survey: Stellar radii in the young open clusters NGC 2264, NGC 2547, and NGC 2516]The Gaia-ESO Survey: Stellar radii in the young open clusters NGC 2264, NGC 2547, and NGC 2516

Delgado, A. J.Sampedro, L.Alfaro, E. J.Costado, M. T.Yun, J. L.Frasca, A.Lanzafame, A. C.Drew, J. E.Eislöffel, J.Blomme, R.Morel, T.Lobel, A.Semaan, T.Randich, S.Jeffries, R. D.Micela, G.Vallenari, A.Kalari, V.Gilmore, G.Flaccomio, E.Carraro, G.Lardo, C.Monaco, L.Prisinzano, L.Sousa, S. G.Morbidelli, L.Lewis, J.Koposov, S.Hourihane, A.Worley, C.Casey, A.Franciosini, E.Sacco, G.Magrini, L.[The Gaia-ESO Survey: pre-main-sequence stars in the young open cluster NGC 3293]The Gaia-ESO Survey: pre-main-sequence stars in the young open cluster NGC 3293

Aims. Carbon-enhanced metal-poor (CEMP) stars represent a sizeable fraction of all known metal-poor stars in the Galaxy. Their formation and composition remains a significant topic of investigation within the stellar astrophysics community. Methods. We analysed a sample of low-resolution spectra ...


Caffau, E.Gallagher, A.J.Bonifacio, P.Spite, M.Duffau, S.Spite, F.Monaco, L.Sbordone, L.[Investigation of a sample of carbon-enhanced metal-poor stars observed with FORS and GMOS]Investigation of a sample of carbon-enhanced metal-poor stars observed with FORS and GMOS

NGC 6791 is a unique stellar cluster, key to our understanding of both the multiple stellar population phenomenon and the evolution and assembly of the Galaxy. However, despite many investigations, its nature is still very controversial. Geisler et al. found evidence suggesting that it was the fi...


Villanova, S.Carraro, G.Geisler, D.Monaco, L.Assmann, P.[NGC 6791: A Probable Bulge Cluster without Multiple Populations]NGC 6791: A Probable Bulge Cluster without Multiple Populations

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